Modeling of kilometer-scale ionospheric irregularities at Mars

Recently, kilometer-scale Martian ionospheric irregularities have been measured by the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission (Fowler et al., 2020). In this study, we carried out a simulation of these irregularities, assuming a uniform Martian zonal neutral wind and a cosinusoidal pe...
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Autor*in:	ChunHua Jiang [verfasserIn] Rong Tian [verfasserIn] LeHui Wei [verfasserIn] GuoBin Yang [verfasserIn] ZhengYu Zhao [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2022

Schlagwörter:	martian ionosphere ionospheric irregularities numerical simulation

Übergeordnetes Werk:	In: Earth and Planetary Physics - Science Press, 2022, 6(2022), 2, Seite 213-217
Übergeordnetes Werk:	volume:6 ; year:2022 ; number:2 ; pages:213-217

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.26464/epp2022011

Katalog-ID:	DOAJ02507668X

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allfields	10.26464/epp2022011 doi (DE-627)DOAJ02507668X (DE-599)DOAJc8a24620c0b64ae197e6aff978de3605 DE-627 ger DE-627 rakwb eng QC801-809 GE1-350 ChunHua Jiang verfasserin aut Modeling of kilometer-scale ionospheric irregularities at Mars 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Recently, kilometer-scale Martian ionospheric irregularities have been measured by the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission (Fowler et al., 2020). In this study, we carried out a simulation of these irregularities, assuming a uniform Martian zonal neutral wind and a cosinusoidal perturbation of the plasma density as the seeding source. Results show that a vertical electric field shear could be induced by such a plasma density perturbation. We find that the vertical electric field shear causes a velocity shear of the plasma between the topside and bottomside ionosphere, which in turn is able to produce kilometer-scale ionospheric irregularities — irregularities of a smaller scale than were seen in previous simulations (Jiang CH et al., 2021). These kilometer-scale variations with altitude, in plasma density and magnetic field profiles, are comparable to the MAVEN observations. martian ionosphere ionospheric irregularities numerical simulation Science Q Geophysics. Cosmic physics Environmental sciences Rong Tian verfasserin aut LeHui Wei verfasserin aut GuoBin Yang verfasserin aut ZhengYu Zhao verfasserin aut In Earth and Planetary Physics Science Press, 2022 6(2022), 2, Seite 213-217 (DE-627)1017742499 20963955 nnns volume:6 year:2022 number:2 pages:213-217 https://doi.org/10.26464/epp2022011 kostenfrei https://doaj.org/article/c8a24620c0b64ae197e6aff978de3605 kostenfrei http://www.eppcgs.org/article/doi/10.26464/epp2022011?pageType=en kostenfrei https://doaj.org/toc/2096-3955 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2031 GBV_ILN_2037 GBV_ILN_2039 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 6 2022 2 213-217
spelling	10.26464/epp2022011 doi (DE-627)DOAJ02507668X (DE-599)DOAJc8a24620c0b64ae197e6aff978de3605 DE-627 ger DE-627 rakwb eng QC801-809 GE1-350 ChunHua Jiang verfasserin aut Modeling of kilometer-scale ionospheric irregularities at Mars 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Recently, kilometer-scale Martian ionospheric irregularities have been measured by the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission (Fowler et al., 2020). In this study, we carried out a simulation of these irregularities, assuming a uniform Martian zonal neutral wind and a cosinusoidal perturbation of the plasma density as the seeding source. Results show that a vertical electric field shear could be induced by such a plasma density perturbation. We find that the vertical electric field shear causes a velocity shear of the plasma between the topside and bottomside ionosphere, which in turn is able to produce kilometer-scale ionospheric irregularities — irregularities of a smaller scale than were seen in previous simulations (Jiang CH et al., 2021). These kilometer-scale variations with altitude, in plasma density and magnetic field profiles, are comparable to the MAVEN observations. martian ionosphere ionospheric irregularities numerical simulation Science Q Geophysics. Cosmic physics Environmental sciences Rong Tian verfasserin aut LeHui Wei verfasserin aut GuoBin Yang verfasserin aut ZhengYu Zhao verfasserin aut In Earth and Planetary Physics Science Press, 2022 6(2022), 2, Seite 213-217 (DE-627)1017742499 20963955 nnns volume:6 year:2022 number:2 pages:213-217 https://doi.org/10.26464/epp2022011 kostenfrei https://doaj.org/article/c8a24620c0b64ae197e6aff978de3605 kostenfrei http://www.eppcgs.org/article/doi/10.26464/epp2022011?pageType=en kostenfrei https://doaj.org/toc/2096-3955 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2031 GBV_ILN_2037 GBV_ILN_2039 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 6 2022 2 213-217
allfields_unstemmed	10.26464/epp2022011 doi (DE-627)DOAJ02507668X (DE-599)DOAJc8a24620c0b64ae197e6aff978de3605 DE-627 ger DE-627 rakwb eng QC801-809 GE1-350 ChunHua Jiang verfasserin aut Modeling of kilometer-scale ionospheric irregularities at Mars 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Recently, kilometer-scale Martian ionospheric irregularities have been measured by the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission (Fowler et al., 2020). In this study, we carried out a simulation of these irregularities, assuming a uniform Martian zonal neutral wind and a cosinusoidal perturbation of the plasma density as the seeding source. Results show that a vertical electric field shear could be induced by such a plasma density perturbation. We find that the vertical electric field shear causes a velocity shear of the plasma between the topside and bottomside ionosphere, which in turn is able to produce kilometer-scale ionospheric irregularities — irregularities of a smaller scale than were seen in previous simulations (Jiang CH et al., 2021). These kilometer-scale variations with altitude, in plasma density and magnetic field profiles, are comparable to the MAVEN observations. martian ionosphere ionospheric irregularities numerical simulation Science Q Geophysics. Cosmic physics Environmental sciences Rong Tian verfasserin aut LeHui Wei verfasserin aut GuoBin Yang verfasserin aut ZhengYu Zhao verfasserin aut In Earth and Planetary Physics Science Press, 2022 6(2022), 2, Seite 213-217 (DE-627)1017742499 20963955 nnns volume:6 year:2022 number:2 pages:213-217 https://doi.org/10.26464/epp2022011 kostenfrei https://doaj.org/article/c8a24620c0b64ae197e6aff978de3605 kostenfrei http://www.eppcgs.org/article/doi/10.26464/epp2022011?pageType=en kostenfrei https://doaj.org/toc/2096-3955 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2031 GBV_ILN_2037 GBV_ILN_2039 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 6 2022 2 213-217
allfieldsGer	10.26464/epp2022011 doi (DE-627)DOAJ02507668X (DE-599)DOAJc8a24620c0b64ae197e6aff978de3605 DE-627 ger DE-627 rakwb eng QC801-809 GE1-350 ChunHua Jiang verfasserin aut Modeling of kilometer-scale ionospheric irregularities at Mars 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Recently, kilometer-scale Martian ionospheric irregularities have been measured by the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission (Fowler et al., 2020). In this study, we carried out a simulation of these irregularities, assuming a uniform Martian zonal neutral wind and a cosinusoidal perturbation of the plasma density as the seeding source. Results show that a vertical electric field shear could be induced by such a plasma density perturbation. We find that the vertical electric field shear causes a velocity shear of the plasma between the topside and bottomside ionosphere, which in turn is able to produce kilometer-scale ionospheric irregularities — irregularities of a smaller scale than were seen in previous simulations (Jiang CH et al., 2021). These kilometer-scale variations with altitude, in plasma density and magnetic field profiles, are comparable to the MAVEN observations. martian ionosphere ionospheric irregularities numerical simulation Science Q Geophysics. Cosmic physics Environmental sciences Rong Tian verfasserin aut LeHui Wei verfasserin aut GuoBin Yang verfasserin aut ZhengYu Zhao verfasserin aut In Earth and Planetary Physics Science Press, 2022 6(2022), 2, Seite 213-217 (DE-627)1017742499 20963955 nnns volume:6 year:2022 number:2 pages:213-217 https://doi.org/10.26464/epp2022011 kostenfrei https://doaj.org/article/c8a24620c0b64ae197e6aff978de3605 kostenfrei http://www.eppcgs.org/article/doi/10.26464/epp2022011?pageType=en kostenfrei https://doaj.org/toc/2096-3955 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2031 GBV_ILN_2037 GBV_ILN_2039 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 6 2022 2 213-217
allfieldsSound	10.26464/epp2022011 doi (DE-627)DOAJ02507668X (DE-599)DOAJc8a24620c0b64ae197e6aff978de3605 DE-627 ger DE-627 rakwb eng QC801-809 GE1-350 ChunHua Jiang verfasserin aut Modeling of kilometer-scale ionospheric irregularities at Mars 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Recently, kilometer-scale Martian ionospheric irregularities have been measured by the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission (Fowler et al., 2020). In this study, we carried out a simulation of these irregularities, assuming a uniform Martian zonal neutral wind and a cosinusoidal perturbation of the plasma density as the seeding source. Results show that a vertical electric field shear could be induced by such a plasma density perturbation. We find that the vertical electric field shear causes a velocity shear of the plasma between the topside and bottomside ionosphere, which in turn is able to produce kilometer-scale ionospheric irregularities — irregularities of a smaller scale than were seen in previous simulations (Jiang CH et al., 2021). These kilometer-scale variations with altitude, in plasma density and magnetic field profiles, are comparable to the MAVEN observations. martian ionosphere ionospheric irregularities numerical simulation Science Q Geophysics. Cosmic physics Environmental sciences Rong Tian verfasserin aut LeHui Wei verfasserin aut GuoBin Yang verfasserin aut ZhengYu Zhao verfasserin aut In Earth and Planetary Physics Science Press, 2022 6(2022), 2, Seite 213-217 (DE-627)1017742499 20963955 nnns volume:6 year:2022 number:2 pages:213-217 https://doi.org/10.26464/epp2022011 kostenfrei https://doaj.org/article/c8a24620c0b64ae197e6aff978de3605 kostenfrei http://www.eppcgs.org/article/doi/10.26464/epp2022011?pageType=en kostenfrei https://doaj.org/toc/2096-3955 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2031 GBV_ILN_2037 GBV_ILN_2039 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 6 2022 2 213-217
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callnumber-first	Q - Science
author	ChunHua Jiang
spellingShingle	ChunHua Jiang misc QC801-809 misc GE1-350 misc martian ionosphere misc ionospheric irregularities misc numerical simulation misc Science misc Q misc Geophysics. Cosmic physics misc Environmental sciences Modeling of kilometer-scale ionospheric irregularities at Mars
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topic_title	QC801-809 GE1-350 Modeling of kilometer-scale ionospheric irregularities at Mars martian ionosphere ionospheric irregularities numerical simulation
topic	misc QC801-809 misc GE1-350 misc martian ionosphere misc ionospheric irregularities misc numerical simulation misc Science misc Q misc Geophysics. Cosmic physics misc Environmental sciences
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title	Modeling of kilometer-scale ionospheric irregularities at Mars
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title_full	Modeling of kilometer-scale ionospheric irregularities at Mars
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title_sort	modeling of kilometer-scale ionospheric irregularities at mars
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title_auth	Modeling of kilometer-scale ionospheric irregularities at Mars
abstract	Recently, kilometer-scale Martian ionospheric irregularities have been measured by the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission (Fowler et al., 2020). In this study, we carried out a simulation of these irregularities, assuming a uniform Martian zonal neutral wind and a cosinusoidal perturbation of the plasma density as the seeding source. Results show that a vertical electric field shear could be induced by such a plasma density perturbation. We find that the vertical electric field shear causes a velocity shear of the plasma between the topside and bottomside ionosphere, which in turn is able to produce kilometer-scale ionospheric irregularities — irregularities of a smaller scale than were seen in previous simulations (Jiang CH et al., 2021). These kilometer-scale variations with altitude, in plasma density and magnetic field profiles, are comparable to the MAVEN observations.
abstractGer	Recently, kilometer-scale Martian ionospheric irregularities have been measured by the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission (Fowler et al., 2020). In this study, we carried out a simulation of these irregularities, assuming a uniform Martian zonal neutral wind and a cosinusoidal perturbation of the plasma density as the seeding source. Results show that a vertical electric field shear could be induced by such a plasma density perturbation. We find that the vertical electric field shear causes a velocity shear of the plasma between the topside and bottomside ionosphere, which in turn is able to produce kilometer-scale ionospheric irregularities — irregularities of a smaller scale than were seen in previous simulations (Jiang CH et al., 2021). These kilometer-scale variations with altitude, in plasma density and magnetic field profiles, are comparable to the MAVEN observations.
abstract_unstemmed	Recently, kilometer-scale Martian ionospheric irregularities have been measured by the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission (Fowler et al., 2020). In this study, we carried out a simulation of these irregularities, assuming a uniform Martian zonal neutral wind and a cosinusoidal perturbation of the plasma density as the seeding source. Results show that a vertical electric field shear could be induced by such a plasma density perturbation. We find that the vertical electric field shear causes a velocity shear of the plasma between the topside and bottomside ionosphere, which in turn is able to produce kilometer-scale ionospheric irregularities — irregularities of a smaller scale than were seen in previous simulations (Jiang CH et al., 2021). These kilometer-scale variations with altitude, in plasma density and magnetic field profiles, are comparable to the MAVEN observations.
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title_short	Modeling of kilometer-scale ionospheric irregularities at Mars
url	https://doi.org/10.26464/epp2022011 https://doaj.org/article/c8a24620c0b64ae197e6aff978de3605 http://www.eppcgs.org/article/doi/10.26464/epp2022011?pageType=en https://doaj.org/toc/2096-3955
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In this study, we carried out a simulation of these irregularities, assuming a uniform Martian zonal neutral wind and a cosinusoidal perturbation of the plasma density as the seeding source. Results show that a vertical electric field shear could be induced by such a plasma density perturbation. We find that the vertical electric field shear causes a velocity shear of the plasma between the topside and bottomside ionosphere, which in turn is able to produce kilometer-scale ionospheric irregularities — irregularities of a smaller scale than were seen in previous simulations (Jiang CH et al., 2021). 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Modeling of kilometer-scale ionospheric irregularities at Mars

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